1980
DOI: 10.1086/372822
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Introduction to Islamic Civilization. R. M. Savory

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Cited by 4 publications
(4 citation statements)
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“…We also use several estimations by Viotti et al [22], and one by Humphreys [29]. They are well consistent with our data.…”
Section: Photometric Observationssupporting
confidence: 91%
See 1 more Smart Citation
“…We also use several estimations by Viotti et al [22], and one by Humphreys [29]. They are well consistent with our data.…”
Section: Photometric Observationssupporting
confidence: 91%
“…A more detailed description of all the photographic data is presented in [16]. We also use several estimations by Viotti et al [22], and one by Humphreys [29]. They are well consistent with our data.…”
Section: Photometric Observationssupporting
confidence: 83%
“…Star-forming regions in the Galaxy and in spirals are most often adjacent to dusty areas that mark molecular clouds (97), so a dearth of dark clouds in star-forming galaxies is unexpected. An exami nation of blue and red passband images, Balmer decrements, and optical and radio-determined star formation rates shows that even in and around star-forming sites, optical interstellar extinction in Irrs tends to be low [maximum E(B-V) � 0.5 (188,191,340) ; fo r the Magellanic Clouds, see, fo r example, 89,111,184,186,234,271]. This may be in part a reflection of the underabundance of heavy elements, which certainly results in some modifications of dust properties (e.g.…”
Section: Star-forming Complexes and The In Terstellar Mediummentioning
confidence: 99%
“…In Μ 31 and Μ 33, the radio emission from SNR is quite weak. As an example, an intense young galactic SNR such as Tycho (3C 10; 43 Jy at a distance of ~ 4 kpc) would have a flux density of only ~ 2 mJy at a distance of 600 kpc corresponding to the distance of Μ 33 (Humphreys 1980). A radio survey of Μ 31 SNR using the VLA has been carried out by Dickel et al (1982), who detected five SNR at 20 cm with flux densities in the range 1 to 3.4 mJy.…”
Section: Introductionmentioning
confidence: 99%